175 citations · 2.6k across the 91 of their papers we have counts for
8 papers · 2 filters
TOI-216: Resonant Constraints on Planet Migration
David Nesvorny, Ondrej Chrenko, Mario Flock
TOI-216 is a pair of close-in planets with orbits deep in the 2:1 mean motion resonance. The inner, Neptune-class planet (TOI-216b) is near 0.12 au (orbital period $P_{\rm b} \sime…
Steady-state accretion in magnetized protoplanetary disks
Timmy N. Delage, Satoshi Okuzumi, Mario Flock +2
[abridged] We present a 1+1D global magnetically-driven disk accretion model that captures the essence of the MRI-driven accretion, without resorting to 3D global non-ideal MHD sim…
The Substructures in Disks undergoing Vertical Shear Instability: II. Observational Predictions for the Dust Continuum
Diana Blanco, Luca Ricci, Mario Flock +1
High-angular resolution observations at sub-millimeter/millimeter wavelengths of disks surrounding young stars have shown that their morphology is made of azimuthally-symmetric or…
Observability of the Vertical Shear Instability in protoplanetary disk CO kinematics
Marcelo Barraza-Alfaro, Mario Flock, Sebastian Marino +1
Context. Dynamical and turbulent motions of gas in a protoplanetary disk are crucial for their evolution and affect planet formation. Recent observations suggest weak turbulence in…
Thermal Wave Instability as an Origin of Gap and Ring Structures in Protoplanetary Disks
Takahiro Ueda, Mario Flock, Tilman Birnstiel
Recent millimeter and infrared observations have shown that gap and ring-like structures are common in both dust thermal emission and scattered-light of protoplanetary disks. We in…
Observable scattered light features from inclined and non-inclined planets embedded in protoplanetary discs
D. Kloster, M. Flock
Over the last few years instruments such as VLT/SPHERE and Subaru/HiCIAO have been able to take detailed scattered light images of protoplanetary discs. Many of the features observ…